Focusing on the study of light unflavor vector meson spectroscopy, we find big progress made by experiment in the past years [1]}, [2]}, [3]}. A typical example is the observation of the \(Y(2175)\)  [4]} and the following measurement [5]}, [6]}, [7]}, [8]}, [9]}, [10]} around the \(Y(2175)\) , which have stimulated extensive discussions of decoding the property of the \(Y(2175)\)  [11]}, [12]}, [13]}, [14]}, [15]}, [16]}. Among these discussions, whether or not the \(Y(2175)\)  can be categorized into \(\phi \)  meson family becomes a long-stranding issue [17]}, [13]}, [19]}. In fact, the light unflavor vector mesons also include these states in the \(\rho \)  and \(\omega \)  meson families. With the accumulation of data with unprecedented statistical accuracy, the \(\rho \)  and \(\omega \)  state around 2 GeV appeared in front of people [20]}, [21]}, [22]}, [23]}, [24]}, [25]}, [26]}, [27]}, [28]}. By the join effort from both theoretical and experimentalist, our knowledge of light unflavor vector meson spectroscopy below 2.2 GeV has been promoted, which is the situation of the study of unflavor vector meson spectroscopy. But, it is not the whole aspect of light unflavor vector meson spectroscopy.
